Space-time picture of hadronic and nuclear collisions

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From low to high energies. Space-time picture of hadronic and nuclear collisions. collision @ alice. collision @ alice. It is essential to understand hadronic interactions at LHC! the structure of the underlying event behaviour of σ tot, σ el and σ diff with energy... - PowerPoint PPT Presentation

Transcript of Space-time picture of hadronic and nuclear collisions

SPACE-TIME PICTURE OF HADRONIC AND NUCLEAR COLLISIONS

From low to high energies

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COLLISION @ ALICE16.05.2008

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COLLISION @ ALICE16.05.2008

Higgs?

junk?

It is essential to understand hadronic interactions at LHC!

the structure of the underlying event

behaviour of σtot, σel and σdiff with energy...

99,9999% of event!! pp interactions at LHC are

small AA systems?

...or else, no discovery!

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OVERVIEW What is a hadron/nucleus? What are

the relevant degrees of freedom? How does a hadron interact with

another hadron? What about nuclei? What is the difference of these

interactions going from low to high energies?

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hadrons, nuclei

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COMPLEX BUILDING BLOCKS

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WHAT IS A HADRON? strongly interacting

composite subatomic particle consists of quarks

baryons: 3 quarks, fermion mesons: quark – anti-quark

pair, boson excited states - resonances at high enough temperatures

they dissolve!

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u

d

u

du

u d

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STRANGE AND STRONG INTERACTION16.05.2008

qq

q q

qq qq

Quantum ChromoDynamics (QCD) – fundamentalo calculable for short distance processeso calculable on lattice for static situationso useless for large distance physics, dynamics...

need approximations, models, ideas!

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NUCLEAR PHYSICS AT HIGH ENERGIES

”macroscopic” volumes conditions ~early Universe free quarks and gluons? Quark-Gluon Plasma (QGP)

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u

du

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HYDRODYNAMICAL PICTURE

need to assume infinitesimally small cells are locally thermalized large rate of interaction

can define temperature, energy density and pressure

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Lev Landau

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THERMALIZATION

usually: particles start with an arbitrary velocity distribution

”equilibrate” over time, maximization of entropy take the continuum limit – loosing the concept

of ”particles”

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0 T

pguupT

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BJORKEN INITIAL CONDITION

boost invariant initial condition, adiabatical expansion

the longitudinal motion is uniform: vz=z/t

gives rise to a central plateau – height independent of energy!

initial energy density

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dydE

RT

Bj0

2

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PICTURE OF A FAST HADRON

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FEYNMANS (NAIVE) PARTON MODEL

• in a frame where the hadron is moving infinitely fast, it consists of infinitely many partons

• the partons carry a fraction of the total momentum of the hadron each

• the partons are free!

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ud

u

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HOW CAN THIS BE?

uncertainty principle! the constituent quarks can

interact via gluon exchange fluctuate into a quark-antiquark pair

when boosting the proton, the timescales related to these fluctuations are Lorentz dilated interactions of quarks now take place over much

larger timescales..

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DISTRIBUTION OF QUARKS AND GLUONS

the probatility of finding a parton (quark, gluon, heavy quark...) with momentum fraction x of the total proton

non-perturbative quantity but dependence on

”resolution” given by QCD

universal quantity measured in ep

collisions can predict νp, pp

etc...

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heavy-ion collisions at RHIC!

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PICTURE OF A FAST HADRON16.05.2008

fast partons

slow partons

target

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12222

mM2ppmpM

ΔE1τ

nxxx ...1 10

1t 2t 3t< <

The lifetime of the fluctuation can be quite large!

Strong ordering from fast to slow partons:

Only correlation between ”nearest neighbours”...

V.N. Gribov

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TRANSVERSE SPACE PICTURE

random walk in the transverse plane each step ~1/μ # of steps ~ln(E)

interaction range

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R

initial parton

target

22 )ln(

ER

“OCTOPUS” PICTURE

yybP y

tsf ee'41),( '42

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PICTURE OF A FAST HADRON16.05.2008

p

Rlog

2|| pR

fast partons- localized in a contracted disc

slow partons- spread out on long itudinal distances

xpplL0

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soft part of the fast hadron is not Lorentz contracted!AT HIGH ENERGY THE PROTON CAN BECOME LARGER THAN A NUCLEUS!

mostly gluons at low-x:

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FROM A NUCLEUS’ POINT OF VIEW...16.05.2008

overlap of nucleons in the nucleus huge density of gluons

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hadron-hadron, hadron-nucleus, nucleus-nucleus

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COLLISIONS

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COMPLICATED PROBLEM

in principle an infinite series need to find the most important terms

single-Pomeron diagram describes existing data quite OK! problems with the theory at high energies,

eg. LHC! need multi-Pomeron exchanges

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...++ ...+

Donnachie, Landshof

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MULTIPERIPHERAL MODEL

the reggeon can be seen as an exchanged ladder of particles in the t-channel

the partons take a fraction ε of the initial energy

#of particles in the fluctuation: n~ln(E) Reggeon is a highly non-local object

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Amati, Fubini, StanghelliniGribov

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IN THE CENTER OF MASS FRAME16.05.2008

single-ladder exchange a large amount of additional particles are created! Feynman-plateau

projectile

target

yy

”central plateu”FIN

AL STATE

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MULTIPLE SCATTERING

1st correction to the single-ladder exchange

”classical” rescattering picture low and intermediate energies –

potential scattering

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THE GLAUBER MODEL16.05.2008

heavy-ion collisions in each rescattering there is a

certain probability for particle production

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THE GLAUBER MODEL16.05.2008

2RA

2RA/γ

# of collisions

xxnxn

xnxddsd

collpart

pp 2)1(

2

3

entropy density related to number of interactions

”initial condition”

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BUT IS THIS PICTURE VALID AT HIGH ENERGIES?

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MULTIPLE LADDER STRUCTURE

at high energies, multiple ladders can start to evolve simultaneously

gives rise to novel physical phenomena

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NON-PLANAR GRAPHS

planar diagram vanishes at high energies ladders require a long time to develop critical energy E0=mNμRA

the projectile goes into a fluctuation long before the collision takes place ladders develop at the same time

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MandelstamGribov

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COHERENT INTERACTION16.05.2008

the projectile becomes large compared to the target

interacts simultaneously with the whole system effectively less interaction - shadowing dramatic change of space-time picture

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CHANGE OF SPACE-TIME PICTURE16.05.2008

the diagrams corresponding to ”classical” rescatterings are suppressed at high energies!

Gribov trick: Glauber is OK after all! Almost... have to take into account diffractive

intermediate states!

E1

(2)totσ + + . . .totσ

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planar diagrams

non-planar

SMOOTH BEHAVIOUR OF OBSERVABLES

the observables don’t feel the change of space-time picture

at high energy: nuclear shadowing are there any observables that are

sensitive to this transition?

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E

|Δσ2|

AN RmE 0

totalσdiffractive

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A1/3Enhanced in AA collisions

CASCADING – ENHANCED DIAGRAMS16.05.2008

k

All particles with can interact. Ο(R)k z

=Triple-Pomeron coupling:quite small or quite large?important at high energiesparton saturation!

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WHAT HAPPENS AT LHC?

interesting physics! probing the strongest force in new

domain! evolution of partons resembles

growth of bacteria colony reaction-diffusion process

striking experimental features!

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OUTLOOK16.05.2008

will large interaction of partons early on prepare a thermalized system in AA? in pp?

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COHERENCE CORRECTIONS

σtot=σ(hp)+σ(hn)=2(σinel+σel)=2Sξ+Sξ2/2

impulse approximation result

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Corrections: loss of flux in the second interaction -Sξ2

contrib to double multiplicity event -Sξ2

contrib to double multiplicity event Sξ2

enhancement of elastic cross section Sξ2/2 12-4

AGK ratios

Bartels, Ryskin Z. Phys. C 76, 241

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22

e)0(1'21

yigxy

L

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mpln)ln( AmR

#par

ticle

s

y

hadron targetnucleus target

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absorption

shadowingE

correction factor

AN RmE 0

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STAGES OF A HEAVY-ION COLLISION16.05.2008

Nuclear GeometryParton distributionsNuclear shadowing

Parton production& reinteraction

Chemical Freeze out &Quark Recombination

Jet FragmentationFunctions

Hadron Rescattering

Thermal Freeze out &Hadron decays

0 fm/c

2 fm/c

7 fm/c

>7 fm/c